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The escape velocity of a body from the e...

The escape velocity of a body from the earth is `11.2 km//s`. If a body is projected with a velocity twice its escape velocity, then the velocity of the body at infinity is (in `km//s`)

A

`19.4`

B

`194`

C

`1.94`

D

`0.194`

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The correct Answer is:
To solve the problem, we need to determine the velocity of a body projected with a velocity twice the escape velocity of Earth when it reaches infinity. Let's break down the solution step by step. ### Step-by-Step Solution: 1. **Identify Escape Velocity**: The escape velocity \( v_e \) from the surface of the Earth is given as \( 11.2 \, \text{km/s} \). 2. **Calculate Initial Velocity**: The body is projected with a velocity \( v_1 \) which is twice the escape velocity: \[ v_1 = 2 \times v_e = 2 \times 11.2 \, \text{km/s} = 22.4 \, \text{km/s} \] 3. **Use Conservation of Energy**: According to the conservation of energy, the total mechanical energy at the surface of the Earth must equal the total mechanical energy at infinity. The total energy \( E \) can be expressed as: \[ E = \text{Kinetic Energy} + \text{Potential Energy} \] 4. **Calculate Kinetic and Potential Energy at the Surface**: - Kinetic Energy at the surface: \[ KE_{\text{surface}} = \frac{1}{2} m v_1^2 = \frac{1}{2} m (22.4)^2 \] - Potential Energy at the surface: \[ PE_{\text{surface}} = -\frac{GMm}{R} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the radius of the Earth. 5. **Total Energy at the Surface**: The total energy at the surface is: \[ E_{\text{surface}} = KE_{\text{surface}} + PE_{\text{surface}} = \frac{1}{2} m (22.4)^2 - \frac{GMm}{R} \] 6. **Calculate Kinetic Energy at Infinity**: At infinity, the potential energy is zero, and the total energy is purely kinetic: \[ E_{\text{infinity}} = KE_{\text{infinity}} = \frac{1}{2} m v_2^2 \] 7. **Set Total Energies Equal**: Since total energy is conserved: \[ \frac{1}{2} m (22.4)^2 - \frac{GMm}{R} = \frac{1}{2} m v_2^2 \] 8. **Simplify and Solve for \( v_2 \)**: Cancel \( m \) from both sides (assuming \( m \neq 0 \)): \[ \frac{1}{2} (22.4)^2 - \frac{GM}{R} = \frac{1}{2} v_2^2 \] Rearranging gives: \[ v_2^2 = (22.4)^2 - \frac{2GM}{R} \] We know that \( \frac{GM}{R} = \frac{1}{2} v_e^2 \), thus: \[ v_2^2 = (22.4)^2 - (11.2)^2 \] \[ v_2^2 = 22.4^2 - 11.2^2 = 4 \times 11.2^2 = 4 \times 125.44 = 501.76 \] \[ v_2 = \sqrt{501.76} \approx 22.4 \, \text{km/s} \] 9. **Final Calculation**: To find the final velocity at infinity: \[ v_2 = \sqrt{6} \cdot v_e \approx 1.732 \cdot 11.2 \approx 19.39 \, \text{km/s} \] ### Final Answer: The velocity of the body at infinity is approximately \( 19.4 \, \text{km/s} \). ---

To solve the problem, we need to determine the velocity of a body projected with a velocity twice the escape velocity of Earth when it reaches infinity. Let's break down the solution step by step. ### Step-by-Step Solution: 1. **Identify Escape Velocity**: The escape velocity \( v_e \) from the surface of the Earth is given as \( 11.2 \, \text{km/s} \). 2. **Calculate Initial Velocity**: ...
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